A dataset provided by the European Space Agency

Name 15645
Title The Identification of Failed Supernovae
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=15645;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-ba9tse3
Author Sand, David J.
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=15645&mission=hst
Publication
  • A Late-time View of the Progenitor Candidates of the Type II-P SN 2009ib and SN 2012ec
  • A Multiepoch X-Ray Study of the Nearby Seyfert 2 Galaxy NGC 7479: Linking Column Density Variability to the Torus Geometry
  • An Early-time Optical and Ultraviolet Excess in the Type-Ic SN 2020oi
  • Digging a little deeper: characterizing three new extreme ULX candidates
  • Dust in the central parsecs of unobscured AGN: more challenges to the torus
  • Explosion sites of SN 1994W-like transients
  • Hubble Space Telescope Imaging Reveals That SN 2015bh Is Much Fainter than Its Progenitor
  • I-band Asymptotic Giant Branch (IAGB) Stars. II. A First Estimate of Their Precision and a Differential Zero Point
  • I-band Asymptotic Giant Branch Stars. I. Exploring a New Standard Candle for the Extragalactic Distance Scale
  • Nothing to see here: failed supernovae are faint or rare
  • Observational Constraints on Cool Gas Clouds in M82s Starburst-driven Outflow
  • Optical Emission from Luminous and Very Soft X-Ray Sources in Nearby Galaxies: Testing the Scenario of Edge-on Supercritical Accretion Systems
  • Photometric and spectroscopic evolution of the interacting transient AT 2016jbu(Gaia16cfr)
  • Progenitor, environment, and modelling of the interacting transient AT 2016jbu (Gaia16cfr)
  • SN 2019ehk: A Double-peaked Ca-rich Transient with Luminous X-Ray Emission and Shock-ionized Spectral Features
  • The Blue Supergiant Progenitor of the Supernova Imposter AT 2019krl
  • The changing-type SN 2014C may come from an 11-M star stripped by binary interaction and violent eruption
  • The impact of satellite trails on Hubble Space Telescope observations
  • The nature of the symbiotic candidate 2MASS J07363415+6538548 in the field of NGC 2403
  • The Type II supernova SN 2020jfo in M 61, implications for progenitor system, and explosion dynamics
  • TRGB Distances to Galaxies Based on Hubble Space Telescope (HST) Images in One F814W Filter1
  • Ultraluminous X-ray sources in seven edge-on spiral galaxies
Instrument ACS/WFC
Temporal Coverage 2019-03-25T06:37:22Z/2019-09-28T20:51:48Z
Version 1.0
Mission Description Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited.
Creator Contact https://support.cosmos.esa.int/esdc/index.php?/Tickets/Submit
Date Published 2020-05-26T00:00:00Z
Last Update 2026-03-09
Keywords Hubble Space Telescope data, HST observations dataset, NASA ESA Hubble mission data, space-based optical imaging data, ultraviolet astronomy observations, near-infrared imaging dataset, Hubble spectroscopy data, Wide Field Camera 3 WFC3 data, Advanced Camera for Surveys ACS data, Space Telescope Imaging Spectrograph STIS data, Cosmic Origins Spectrograph COS data, Hubble deep field imaging dataset, extragalactic survey observations, galaxy evolution imaging data, star formation observations HST, stellar photometry dataset, globular cluster imaging data, supernova Hubble observations, exoplanet transit HST data, interstellar medium spectroscopy data, calibrated level 2 HST data products, drizzled image mosaics, FITS files astronomy, flux-calibrated spectra, photometric time-series Hubble data, redshift measurements dataset, Hubble Legacy Archive data, Mikulski Archive for Space Telescopes MAST dataset
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Sand et al., 2020, 'The Identification of Failed Supernovae', 1.0, European Space Agency, https://doi.org/10.5270/esa-ba9tse3